Atmospheric Neutrino Mixing and b-s Transitions: Testing Lopsided SO(10) Flavor Structure in B physics

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dc.creatorJi, Xiangdong
dc.creatorLi, Yingchuan
dc.creatorZhang, Yue
dc.date2006-12-11
dc.date2007-03-04
dc.date.accessioned2026-07-07T10:37:35Z
dc.date.available2026-07-07T10:37:35Z
dc.descriptionWe point out that the correlation between the large atmospheric neutrino mixing and the $b \to s$ transition, if exists, comes from the lopsided flavor structure in SO(10) grand unification theory. We suggest testing the correlation by studying the deviation of $S_{ϕK_S}$ and $S_{η' K_S}$ from the standard model predictions along with the constraints from $ΔM_{B_S}$ and $b\to s γ$ in a realistic SO(10) model with lopsided flavor structure. We find a specific correlation between $S_{ϕK_S}$ and $S_{η' K_S}$ that is intrinsic to the lopsided structure and discuss how to confirm or rule out this flavor pattern by the more accurate measurements of these CP violation quantities in B decay.
dc.description6 pages, 4 figures
dc.identifierhttps://arxiv.org/abs/hep-ph/0612114
dc.identifierhttp://arxiv.org/abs/hep-ph/0612114
dc.identifierPhys.Rev.D75:055016,2007
dc.identifierdoi:10.1103/PhysRevD.75.055016
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/180427
dc.subjectHigh Energy Physics - Phenomenology
dc.titleAtmospheric Neutrino Mixing and b-s Transitions: Testing Lopsided SO(10) Flavor Structure in B physics
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